We develop a compressible liquid-drop model to describe the crust of neutron stars for which the role of the nuclear clusters, the neutron gas, and the ele
Answer to: In the ground state of an atom the electron is present: (a) In the nucleus. (b) In the second shell. (c) Nearest the nucleus. (d)...
A static chem- ical control of the charge state of NV colour centres in diamond has recently been shown13–15. For instance, control of the Fermi energy was achieved by exploiting surface transfer doping in hydro- gen (H)-terminated diamond24. In this case, atmospheric adsorb- ates on the...
The importance of final state interactions between the outgoing nucleon and the residual nucleus is studied with particular emphasis on the relative cross sections for the reactions A( π +, πN) and A( π , πN) and also for the reactions A( π , π n) and A( π , π p) which ...
Here, β≥0 characterises the steady-state with the relative precision (i.e., negative entropy) of policies and final outcomes, given final states. The generative model stipulates steady-state, in the sense that distribution over final states (and outcomes) does not depend upon initial observatio...
A system of particles is said to be in a bound state if the relative motion of the particles occurs in a bounded region of space (is finite) over a period that is long compared with the periods characteristic of the given system. Nature offers many examples of bound states—from star ...
The study of the nuclear matter equation-of-state (EoS) is a relevant topic of modern nuclear physics. It governs the behaviour of nuclear matter away from the normal conditions found in nuclei interiors and plays a major role in heavy-ion collisions, in determining neutron skin thicknesses of...
摘要: How the strong interaction binds the ingredients(proton and neutron)of atomic nuclei,is the central quest of nuclear physics.Nuclear physicists have been addressing this question with different experimental techniques and theoretical approaches.关键词:...
They have been carried out at different chemical-physical conditions and by the use of a number of different approaches, including atomic force microscopy, neutron and X-ray scattering, dynamic light scattering, differential scanning calorimetry, surface quartz microbalance, nuclear magnetic resonance, ...
Recently, there has been rapid development in the field of gravitational wave astronomy, which has provided us with new insights into compact objects such as the black holes (BHs) and the neutron stars (NSs) [1,2,3]. The advancements in gravitational wave detection technology have also made ...